Is the B[e] Star V2028 Cyg a Binary?
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F12%3A10130335" target="_blank" >RIV/00216208:11320/12:10130335 - isvavai.cz</a>
Alternative codes found
RIV/67985815:_____/12:00388458
Result on the web
—
DOI - Digital Object Identifier
—
Alternative languages
Result language
angličtina
Original language name
Is the B[e] Star V2028 Cyg a Binary?
Original language description
V2028 Cyg shows a B[e] phenomenon. Due to the presence of both cool (K7III) and hot (B4III) components in the spectra, it is supposed to be a binary. Our modelling of the time variability of H alpha line bisectors shows, however, that this hybrid spectrum can originate in one star, which is surrounded by a disc.
Czech name
—
Czech description
—
Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
—
Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
FROM INTERACTING BINARIES TO EXOPLANETS: ESSENTIAL MODELING TOOLS
ISBN
978-1-107-01982-9
ISSN
1743-9213
e-ISSN
—
Number of pages
2
Pages from-to
309-310
Publisher name
CAMBRIDGE UNIV PRESS, THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND
Place of publication
Cambridge, UK
Event location
Tatranska Lominica, SLOVAKIA
Event date
Jul 18, 2011
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000309244400089